Design Considerations for an Optical PSK Homodyne Receiver

This thesis presents studies concerned with the design of an optical homodyne PSK receiver. Fundamental receiver sensitivities for a number of optical detection schemes are presented. The principal of performance degradation due to finite phase error in the detection process is established. The major noise source in semiconductor lasers is considered, lineshape anomalies, which may affect coherent communication systems, outlined, and methods for laser phase noise reduction discussed. An experimental technique for the measurement of laser phase noise is implemented, and results from free running lasers presented. Techniques for linewidth reduction are investigated and results given. An analysis of the optical Costas loop, an optimum solution of PSK detection, is presented. Performance in the presence of non-negligible phase noise is considered. Equivalent noise bandwidth integrals are evaluated for a number of loop filter functions, and a design procedure for a second order loop incorporating an active lead-lag filter derived. Consideration is then given to system operation in the presence of significant loop propagation delay. A model of the system is developed and results presented for beat linewidths typical of a number of common laser sources. A number of components necessary for the implementation of the Costas loop are developed. These include a wideband detector/amplifier module, and a phase modulator. Consideration is also given to the design of a 9

High Speed Integrated Circuits for High Speed Coherent Optical Communications

With the development of (sub) THz transistor technologies, high speed integrated circuits up to sub-THz frequencies are now feasible. These high speed and wide bandwidth ICs can improve the performance of optical components, coherent optical fiber communication, and imaging systems. In current optical systems, electrical ICs are used primarily as driving amplifiers for optical modulators, and in receiver chains including TIAs, AGCs, LPFs, ADCs and DSPs. However, there are numerous potential applications in optics using high speed ICs, and different approaches may be required for more efficient, compact and flexible optical systems.This dissertation will discuss three different approaches for optical components and communication systems using high speed ICs: a homodyne optical phase locked loop (OPLL), a heterodyne OPLL, and a new WDM receiver architecture.The homodyne OPLL receiver is designed for short-link optical communication systems using coherent modulation for high spectral efficiency. The phase-locked coherent receiver can recover the transmitted data without requiring complex back-end digital signal processing to recover the phase of the received optical carrier. The main components of the homodyne OPLL are a photonic IC (PIC), an electrical IC (EIC), and a loop filter. One major challenge in OPLL development is loop bandwidth; this must be of order 1 GHz in order for the loop to adequately track and suppress the phase fluctuations of the locked laser, yet a 1 GHz loop bandwidth demands small (<100 ps) propagation delays if the loop is to be stable. Monolithic integration of the high-speed loop components into one electrical and one photonic IC decreases the total loop delay. We have designed and demonstrated an OPLL with a compact size of 10 × 10 mm2, stably operating with a loop bandwidth of 1.1 GHz, a loop delay of 120 ps, a pull-in time of 0.55 μs and lock time of <10 ns. The coherent receiver can receive 40 Gb/s BPSK data with a bit error rate (BER) of <10-7, and operates up to 35 Gb/s with BER 10-12.The thesis also describes heterodyne OPLLs. These can be used to synthesize optical wavelengths of a broad bandwidth (optical wavelength synthesis) with narrow linewidth and with fast frequency switching. There are many applications of such narrow linewidth optical signal sources, including low phase noise mm-wave and THz-signal sources, wavelength-division-multiplexed optical transmitters, and coherent imaging and sensor systems. The heterodyne OPLL also has the same stability issues (loop delay and sensitivity) as the homodyne OPLL. In the EIC, a single sideband mixer operating using digital design principles (DSSBM) enables precisely controlled sweeping of the frequency of the locked laser, with control of the sign of the frequency offset. The loop's phase and frequency difference detector (PFD) uses digital design techniques to make the OPLL loop parameters only weakly sensitive to optical signal levels or optical or electrical component gains. The heterodyne OPLL operates stably with a loop bandwidth of 550 MHz and loop delay of <200 ps. An initial OPLL design exhibited optical frequency (wavelength) synthesis from -6 GHz to -2 GHz and from 2 GHz to 9 GHz. An improved OPLL reached frequency tuning up to 25 GHz. The homodyne OPLL exhibits -110 dBc/Hz phase noise at 10 MHz offset and -80 dBc/Hz at 5 kHz offset.Finally, the thesis describes a new WDM receiver architecture using broadband electrical ICs. In the proposed WDM receiver, a set of received signals at different optical wavelengths are mixed against a single optical local oscillator. This mixing converts the WDM channels to electrical signals in the receiver photocurrent, with each WDM signal being converted to an RF sub-carrier of different frequency. An electrical IC then separately converts each sub-carrier signal to baseband using single-sideband mixers and quadrature local oscillators. The proposed receiver needs less complex hardware than the arrays of wavelength-sensitive receivers now used for WDM, and can readily adjust to changes in the WDM channel frequencies. The proposed WDM receiver concept was demonstrated through several system experiments. Image rejection of greater than 25 dB, adjacent channel suppression of greater than 20 dB, operation with gridless channels, and six-channel data reception at a total 15 Gb/s (2.5 Gb/s BPSK × 6-channels) were demonstrated

An Optomechanical Oscillator on a Silicon Chip

The recent observation on radiation-pressure-driven self-sustained oscillation in high-Q optical microresonators has created new possibilities for development of photonic devices that benefit from unique functionalities offered by these “optomechanical oscillators” (OMOs). Here, we review the physics, fundamental characteristics, and potential applications of OMOs using the silica microtoroidal OMO as an example

Convergence of millimeter-wave and photonic interconnect systems for very-high-throughput digital communication applications

In the past, radio-frequency signals were commonly used for low-speed wireless electronic systems, and optical signals were used for multi-gigabit wired communication systems. However, as the emergence of new millimeter-wave technology introduces multi-gigabit transmission over a wireless radio-frequency channel, the borderline between radio-frequency and optical systems becomes blurred. As a result, there come ample opportunities to design and develop next-generation broadband systems to combine the advantages of these two technologies to overcome inherent limitations of various broadband end-to-end interconnect systems in signal generation, recovery, synchronization, and so on. For the transmission distances of a few centimeters to thousands of kilometers, the convergence of radio-frequency electronics and optics to build radio-over-fiber systems ushers in a new era of research for the upcoming very-high-throughput broadband services. Radio-over-fiber systems are believed to be the most promising solution to the backhaul transmission of the millimeter-wave wireless access networks, especially for the license-free, very-high-throughput 60-GHz band. Adopting radio-over-fiber systems in access or in-building networks can greatly extend the 60-GHz signal reach by using ultra-low loss optical fibers. However, such high frequency is difficult to generate in a straightforward way. In this dissertation, the novel techniques of homodyne and heterodyne optical-carrier suppressions for radio-over-fiber systems are investigated and various system architectures are designed to overcome these limitations of 60-GHz wireless access networks, bringing the popularization of multi-gigabit wireless networks to become closer to the reality. In addition to the advantages for the access networks, extremely high spectral efficiency, which is the most important parameter for long-haul networks, can be achieved by radio-over-fiber signal generation. As a result, the transmission performance of spectrally efficient radio-over-fiber signaling, including orthogonal frequency division multiplexing and orthogonal wavelength division multiplexing, is broadly and deeply investigated. On the other hand, radio-over-fiber is also used for the frequency synchronization that can resolve the performance limitation of wireless interconnect systems. A novel wireless interconnects assisted by radio-over-fiber subsystems is proposed in this dissertation. In conclusion, multiple advantageous facets of radio-over-fiber systems can be found in various levels of end-to-end interconnect systems. The rapid development of radio-over-fiber systems will quickly change the conventional appearance of modern communications.PhDCommittee Chair: Gee-Kung Chang; Committee Member: Bernard Kippelen; Committee Member: Shyh-Chiang Shen; Committee Member: Thomas K. Gaylord; Committee Member: Umakishore Ramachandra

Enabling Technologies for Optical Data Center Networks: Spatial Division Multiplexing

With the continuously growing popularity of cloud services, the traffic volume inside the\ua0data\ua0centers is dramatically increasing. As a result, a scalable and efficient infrastructure\ua0for\ua0data\ua0center\ua0networks\ua0(DCNs) is required. The current\ua0optical\ua0DCNs using either individual fibers or fiber ribbons are costly, bulky, hard to manage, and not scalable.\ua0Spatial\ua0division\ua0multiplexing\ua0(SDM) based on multicore or multimode (few-mode) fibers is recognized as a promising technology to increase the\ua0spatial\ua0efficiency\ua0for\ua0optical\ua0DCNs, which opens a new way towards high capacity and scalability. This tutorial provides an overview of the components, transmission options, and interconnect architectures\ua0for\ua0SDM-based DCNs, as well as potential technical challenges and future directions. It also covers the co-existence of SDM and other\ua0multiplexing\ua0techniques, such as wavelength-division\ua0multiplexing\ua0and flexible spectrum\ua0multiplexing, in\ua0optical\ua0DCNs

Quantum Communication, Sensing and Measurement in Space

The main theme of the conclusions drawn for classical communication systems operating at optical or higher frequencies is that there is a well‐understood performance gain in photon efficiency (bits/photon) and spectral efficiency (bits/s/Hz) by pursuing coherent‐state transmitters (classical ideal laser light) coupled with novel quantum receiver systems operating near the Holevo limit (e.g., joint detection receivers). However, recent research indicates that these receivers will require nonlinear and nonclassical optical processes and components at the receiver. Consequently, the implementation complexity of Holevo‐capacityapproaching receivers is not yet fully ascertained. Nonetheless, because the potential gain is significant (e.g., the projected photon efficiency and data rate of MIT Lincoln Laboratory's Lunar Lasercom Demonstration (LLCD) could be achieved with a factor‐of‐20 reduction in the modulation bandwidth requirement), focused research activities on ground‐receiver architectures that approach the Holevo limit in space‐communication links would be beneficial. The potential gains resulting from quantum‐enhanced sensing systems in space applications have not been laid out as concretely as some of the other areas addressed in our study. In particular, while the study period has produced several interesting high‐risk and high‐payoff avenues of research, more detailed seedlinglevel investigations are required to fully delineate the potential return relative to the state‐of‐the‐art. Two prominent examples are (1) improvements to pointing, acquisition and tracking systems (e.g., for optical communication systems) by way of quantum measurements, and (2) possible weak‐valued measurement techniques to attain high‐accuracy sensing systems for in situ or remote‐sensing instruments. While these concepts are technically sound and have very promising bench‐top demonstrations in a lab environment, they are not mature enough to realistically evaluate their performance in a space‐based application. Therefore, it is recommended that future work follow small focused efforts towards incorporating practical constraints imposed by a space environment. The space platform has been well recognized as a nearly ideal environment for some of the most precise tests of fundamental physics, and the ensuing potential of scientific advances enabled by quantum technologies is evident in our report. For example, an exciting concept that has emerged for gravity‐wave detection is that the intermediate frequency band spanning 0.01 to 10 Hz—which is inaccessible from the ground—could be accessed at unprecedented sensitivity with a space‐based interferometer that uses shorter arms relative to state‐of‐the‐art to keep the diffraction losses low, and employs frequency‐dependent squeezed light to surpass the standard quantum limit sensitivity. This offers the potential to open up a new window into the universe, revealing the behavior of compact astrophysical objects and pulsars. As another set of examples, research accomplishments in the atomic and optics fields in recent years have ushered in a number of novel clocks and sensors that can achieve unprecedented measurement precisions. These emerging technologies promise new possibilities in fundamental physics, examples of which are tests of relativistic gravity theory, universality of free fall, frame‐dragging precession, the gravitational inverse‐square law at micron scale, and new ways of gravitational wave detection with atomic inertial sensors. While the relevant technologies and their discovery potentials have been well demonstrated on the ground, there exists a large gap to space‐based systems. To bridge this gap and to advance fundamental‐physics exploration in space, focused investments that further mature promising technologies, such as space‐based atomic clocks and quantum sensors based on atom‐wave interferometers, are recommended. Bringing a group of experts from diverse technical backgrounds together in a productive interactive environment spurred some unanticipated innovative concepts. One promising concept is the possibility of utilizing a space‐based interferometer as a frequency reference for terrestrial precision measurements. Space‐based gravitational wave detectors depend on extraordinarily low noise in the separation between spacecraft, resulting in an ultra‐stable frequency reference that is several orders of magnitude better than the state of the art of frequency references using terrestrial technology. The next steps in developing this promising new concept are simulations and measurement of atmospheric effects that may limit performance due to non‐reciprocal phase fluctuations. In summary, this report covers a broad spectrum of possible new opportunities in space science, as well as enhancements in the performance of communication and sensing technologies, based on observing, manipulating and exploiting the quantum‐mechanical nature of our universe. In our study we identified a range of exciting new opportunities to capture the revolutionary capabilities resulting from quantum enhancements. We believe that pursuing these opportunities has the potential to positively impact the NASA mission in both the near term and in the long term. In this report we lay out the research and development paths that we believe are necessary to realize these opportunities and capitalize on the gains quantum technologies can offer

Ultralow noise pre-amplified receiver for free-space optical communications

The demand for high data rate in space communication links is increasing due to the growth of space exploration missions inter-satellite, and satellite-to-Earth data transmission. Optical communication systems capable of handling hundreds of Gigabits per second data transmission with a single light carrier and are suitable for such space links. In addition, light offers smaller beam divergence in space due to the shorter wavelength compared to radio frequency beams (RF), resulting in smaller link loss and smaller size receiver apertures required.The receiver sensitivity is one of the key factors that determines the capacity and reach for such long haul communication links. Currently, there is a search for the optimal modulation format and receiver implementation combination to achieve the best sensitivity for error-free transmission. In this thesis, we discuss and implement the best possible combination of these, both theoretically and experimentally. Phase sensitive parametric optical amplifier (PSA) can amplify optical signals ideally without adding any excess noise, limited only by quantum fluctuations. Employing these as preamplifiers in free-space receivers can thus improve the sensitivity compared to erbium doped fiber amplifiers. We implement a two-mode PSA with a noise figure of 1.2 dB, which can amplify both quadratures of a signal, being used as a pre-amplifier in coherent receiver setup. We experimentally demonstrate a record black-box sensitivity of 1 photon-per-bit using PSA receiver for quadrature phase shift keying (QPSK) modulation format at 10.5 Gbps with 100 % overhead forward error correction code. This sensitivity also includes ultra-low pump power (-72 dBm) which is recovered using pre-amplified injection locking. We also investigate the most power efficient modulation formats, where a combination of m-(pulse-position modulation) PPM+QPSK with higher m-values provides best sensitivity at relatively high received SNR-per-bit, while QPSK outperforms all formats investigated at very low SNR-per-bit, which is ideal for space communications